Syllabus topics (official RTMNU)
(A) Atomic structure
- Bohr model, Idea of de-Broglie matter Waves, Heisenberg's uncertainty principle.
- Schrodinger wave equation, significance of ψ and ψ2, Quantum numbers, Concept of atomic orbital, Radial and angular wave functions and probability distribution curves for 1s, 2s, 2p, 3s, 3p and 3d orbitals, shapes of s, p and d orbitals, Aufbau principle, Bohr-Bury rule, Pauli's exclusion principle and Hund's rule of maximum multiplicity.
- Principle of extra stability.
- Electronic Configuration of elements and ions.
(B) Periodic Properties
- Atomic and ionic radii, ionization energy, electron affinity and electronegativity- Definition, trends in periodic table.
- Factors affecting ionization potential.
- Pauling's, Mulliken's and Allred-Rochow scale of electronegativity.
- Effective nuclear charge and Slater's rule with some numericals.
(A) Atomic structure: Bohr model to quantum model
Bohr model (1913)
- Postulate 1: electrons revolve around the nucleus in fixed circular orbits called stationary states or energy levels (n = 1, 2, 3…). In these orbits they do not radiate energy.
- Postulate 2: angular momentum is quantised: mvr = nh/2π.
- Postulate 3: energy is absorbed or emitted only when an electron jumps from one orbit to another: ΔE = E₂ − E₁ = hν.
- Results for hydrogen-like species: rₙ = 0.529 n²/Z Å and Eₙ = −13.6 Z²/n² eV (−2.18 × 10⁻¹⁸ Z²/n² J).
- Limitations: works only for one-electron species (H, He⁺, Li²⁺); cannot explain spectra of multi-electron atoms, fine structure, Zeeman and Stark effects; goes against the uncertainty principle (fixed path).
de Broglie matter waves (1924)
Every moving particle has a wave nature. Wavelength λ = h/mv = h/p. For an electron in a Bohr orbit, a stable orbit holds a whole number of waves: 2πr = nλ, which gives back mvr = nh/2π. The wave nature is noticeable only for very small particles (electrons), not for a cricket ball.
Heisenberg's uncertainty principle (1927)
It is impossible to measure the exact position and exact momentum of a microscopic particle at the same time: Δx · Δp ≥ h/4π. So we cannot speak of a fixed orbit; we can only speak of the probability of finding the electron.
Schrödinger wave equation and orbitals
Schrödinger treated the electron as a 3-D standing wave:
∂²ψ/∂x² + ∂²ψ/∂y² + ∂²ψ/∂z² + (8π²m/h²)(E − V)ψ = 0 (short form Ĥψ = Eψ)
- ψ (wave function): amplitude of the electron wave; it can be +, − or zero and has no physical meaning by itself.
- ψ²: probability density, i.e. probability of finding the electron per unit volume at a point (Born interpretation). It is always positive.
- Acceptable ψ must be single-valued, finite, continuous, and normalised (∫ψ² dτ = 1).
- Atomic orbital: the region around the nucleus where the probability of finding the electron is maximum (about 90–95 %). It is a solution ψ of the wave equation with definite n, l, m.
Quantum numbers
| Quantum number | Values | Tells us |
|---|---|---|
| Principal (n) | 1, 2, 3… | shell, size and energy of orbital |
| Azimuthal (l) | 0 to (n−1) | subshell and shape (l = 0 s, 1 p, 2 d, 3 f); orbital angular momentum √l(l+1)·h/2π |
| Magnetic (m or mₗ) | −l … 0 … +l | orientation in space; number of orbitals = 2l + 1 |
| Spin (s or mₛ) | +½, −½ | spin of electron (clockwise / anticlockwise) |
Radial and angular wave functions; probability curves
ψ is written as ψ(r, θ, φ) = R(r) · Y(θ, φ). R(r) is the radial part (depends on n and l) and Y is the angular part (depends on l and m; decides shape).
- Radial probability distribution = 4πr²R² plotted against r. It shows the probability of finding the electron in a thin spherical shell at distance r.
- Radial nodes = n − l − 1; angular nodes = l; total nodes = n − 1.
- 1s: one peak, maximum at 0.529 Å (Bohr radius), no node.
- 2s: two peaks (small inner, large outer), one radial node. 3s: three peaks, two nodes.
- 2p: one peak, no radial node. 3p: two peaks, one radial node.
- 3d: one peak, no radial node (n − l − 1 = 0), lies closer to nucleus than 3s/3p main peaks.
- The small inner peaks of s orbitals show penetration towards the nucleus, so for the same n the order of energy is s < p < d.
Shapes of orbitals
- s: spherical, non-directional.
- p (pₓ, p_y, p_z): dumb-bell shaped, two lobes with a nodal plane through the nucleus.
- d: five orbitals. d_xy, d_yz, d_zx have four lobes between the axes; d_x²−y² has four lobes along the x and y axes; d_z² has two lobes along z with a ring (doughnut) in the xy plane.
Rules for filling electrons
- Aufbau principle: orbitals are filled in order of increasing energy. (n + l) rule: lower n + l fills first; if equal, lower n fills first. Order: 1s 2s 2p 3s 3p 4s 3d 4p 5s 4d 5p 6s 4f 5d 6p…
- Bohr–Bury rule: maximum electrons in a shell = 2n²; the outermost shell cannot have more than 8 and the penultimate not more than 18 electrons.
- Pauli's exclusion principle: no two electrons in an atom can have all four quantum numbers the same. So one orbital holds maximum 2 electrons with opposite spins.
- Hund's rule of maximum multiplicity: in degenerate orbitals, pairing starts only after each orbital has one electron with parallel spin. Example N: 2p³ = ↑ ↑ ↑ (three unpaired electrons).
Extra stability of half-filled and completely filled subshells
Due to symmetrical distribution and maximum exchange energy, d⁵, d¹⁰, f⁷, f¹⁴ are extra stable. Examples: Cr (24) = [Ar] 3d⁵ 4s¹ (not 3d⁴ 4s²); Cu (29) = [Ar] 3d¹⁰ 4s¹.
Electronic configuration of ions
For cations of transition metals, electrons are removed first from the outer 4s, then 3d. Fe (26) = [Ar] 3d⁶ 4s²; Fe²⁺ = [Ar] 3d⁶; Fe³⁺ = [Ar] 3d⁵ (extra stable, so Fe³⁺ is more stable than Fe²⁺). Anions add electrons: Cl⁻ = [Ne] 3s² 3p⁶.
(B) Periodic properties
| Property | Definition | Across a period (→) | Down a group (↓) |
|---|---|---|---|
| Atomic radius | distance from nucleus to outermost electron (covalent, metallic or van der Waals radius) | decreases | increases |
| Ionic radius | radius of ion in an ionic crystal; cation < parent atom < anion | decreases (isoelectronic: more Z, smaller) | increases |
| Ionisation energy (IE) | energy needed to remove the outermost electron from an isolated gaseous atom: M(g) → M⁺(g) + e⁻ | increases (with exceptions) | decreases |
| Electron affinity (EA) | energy released when an electron is added to an isolated gaseous atom: X(g) + e⁻ → X⁻(g) | increases | decreases (Cl > F because F is very small) |
| Electronegativity (EN) | tendency of an atom in a molecule to attract the shared pair towards itself | increases | decreases |
Factors affecting ionisation potential
- Atomic size: larger size → lower IE.
- Nuclear charge: higher effective nuclear charge → higher IE.
- Screening (shielding) by inner electrons → lower IE.
- Penetration: s > p > d > f; an s electron is harder to remove.
- Stable configuration: half-filled/fully filled shells have high IE. So IE of N > O and Be > B; noble gases highest.
Electronegativity scales
- Pauling scale: from bond energies. Δ = E(A–B) − √[E(A–A) × E(B–B)]; χA − χB = 0.102 √Δ (Δ in kJ mol⁻¹) [or 0.208 √Δ with Δ in kcal mol⁻¹]. F = 4.0 (highest).
- Mulliken scale: average of IE and EA: χ = (IE + EA)/2. With values in eV, χ(Pauling) ≈ χ(Mulliken)/2.8.
- Allred–Rochow scale: EN is the electrostatic force exerted by the nucleus on a valence electron at the covalent radius: χ = 0.359 Z_eff/r² + 0.744 (r = covalent radius in Å).
Effective nuclear charge and Slater's rules
Z_eff = Z − σ, where σ = screening constant. Slater's rules: write groups (1s)(2s,2p)(3s,3p)(3d)(4s,4p)(4d)…
- Electrons to the right of the chosen electron: 0.
- For an ns/np electron: others in the same group 0.35 each (0.30 for 1s); (n−1) shell 0.85 each; (n−2) and lower 1.00 each.
- For a d or f electron: same group 0.35; all electrons to the left 1.00.
Numerical 2: Z_eff for 2p electron of N (Z = 7), (1s²)(2s²2p³). σ = 4 × 0.35 + 2 × 0.85 = 3.1. Z_eff = 7 − 3.1 = 3.9.
Numerical 3: 3d electron of Zn (Z = 30), (1s²)(2s²2p⁶)(3s²3p⁶)(3d¹⁰)(4s²). σ = 9 × 0.35 + 18 × 1.00 = 21.15. Z_eff = 8.85.
Likely exam questions
Long answer
- Explain the significance of ψ and ψ². Draw and discuss the radial probability distribution curves for 1s, 2s, 2p, 3s, 3p and 3d orbitals.
- Define electronegativity. Describe the Pauling, Mulliken and Allred–Rochow scales of electronegativity.
Short answer
- State Heisenberg's uncertainty principle and give its mathematical form.
- State Aufbau principle, Pauli's exclusion principle and Hund's rule with one example each.
- Calculate the effective nuclear charge for the 4s electron of potassium using Slater's rules.